T167 The Evolution of Continental Weathering through Geologic Time: Paleoclimate, Biogeochemistry, Diagenesis, and Clay Minerals
Tuesday, 6 November 2018
8:00 AM - 12:00 PM
Sagamore Ballroom 7
THE CLAY MINERALOGY OF PALEOSOLS IN THE CHINLE FORMATION AT PETRIFIED NATIONAL FOREST: INSIGHTS INTO WEATHERING AND CLIMATE DURING THE LATE TRIASSIC
Paper number: T167-13
Program: Technical Sessions
Time: 10:50 AM – 11:05 AM
Authors
-
Steve I. DworkinBaylor University, Waco, TX
-
Lee C. NordtBaylor University, Waco, TX
-
Stacy AtchleyBaylor University, Waco, TX
Abstract
Clays make up an average of 65% of Chinle paleosols and include the following clays in decreasing order of abundance: mixed layer illite/smectite, illite-mica, kaolinite, palygorskite, and chlorite. The basal portion of the Chinle contains abundant neoformed kaolinite comprising 11% of the whole rock whereas in the upper Chinle kaolinite is almost absent. The sudden loss of kaolinite in paleosols younger than 215 Ma reflects a climate shift involving increased aridity. Further up section, palygorskite comprises 5% of uppermost Chinle paleosols indicating a continuing decline in precipitation as western Pangaean environments evolved into a desert during the Jurassic. The pedogenic threshold from kaolinite to smectite occurs around 1000 mm of precipitation in modern environments and palygorskite formation is restricted to areas with MAP less than 300 mm/yr. Mixed layer illite-smectite is the most abundant clay mineral in Chinle paleosols. The proportion of illite to smectite interlayers decreases up-section, averaging 24% illite layers. The results of the study support the assertion that quantitative x-ray diffraction analysis of clay minerals in paleosols can be a powerful tool for understanding climate controlled chemical reactions.
Geological Society of America Abstracts with Programs. Vol. 50, No. 6
doi: 10.1130/abs/2018AM-322810
© Copyright 2018 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.